collaborators

5 papers

astro-ph.IM2026

Guangqi: A two-dimensional radiation hydrodynamic code with realistic equation of states

Zhuo Chen, Xue-Ning Bai

We present Guangqi, a new two-dimensional, finite-volume radiation hydrodynamics code designed for high-performance astrophysical simulations. The code simultaneously resolves the…

astro-ph.HE2026

Cosmic Ray Magnetohydrodynamics: A New Two-Moment Framework with Numerical Implementation

Xihui Zhao, Xue-Ning Bai, Eve C. Ostriker

Cosmic rays (CRs) play a pivotal role in various astrophysical systems, delivering feedback over a broad range of scales. However, modeling CR transport remains challenging due to…

astro-ph.HE2025

Magnetohydrodynamic-guiding-center-particle-in-cell Method for Multiscale Plasma Kinetic Simulations

Zitao Hu, Xue-Ning Bai, Xiaochen Sun

We present the formulation, algorithm and numerical tests of the magnetohydrodynamic-particle-in-cell (MHD-PIC) method with particles treated under the guiding center approximation…

astro-ph.HE2025

Kinetic simulations of the cosmic ray pressure anisotropy instability: cosmic ray scattering rate in the saturated state

Xiaochen Sun, Xue-Ning Bai, Xihui Zhao

Cosmic ray (CR) feedback plays a vital role in shaping the formation and evolution of galaxies through their interaction with magnetohydrodynamic waves. In the CR self-confinement…

astro-ph.HE2025

Linear Analysis and Simulations of the Cosmic-Ray Streaming Instability: the Importance of Oblique Waves

Shuzhe Zeng, Xue-Ning Bai, Xiaochen Sun

Cosmic-ray (CR) streaming instability (CRSI) is believed to play an important role in CR transport and CR feedback to galaxies. It drives the growth of magnetohydrodynamic (MHD) wa…